Ruprecht 103
(OCL 876; ESO 130 11; MWSC 2012)
Summary
Ruprecht 103 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, above the mid-plane. It is rarely studied in the literature, with no articles listed in the last 6 years.
Warning: contains less than 25 stars with P>0.5 estimated.
Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicates that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Kharchenko et al. (2012) | 184.23 | -58.417 | – | -13.24 | -0.94 | – |
| Bica et al. (2019) | 183.974 | -58.42 | – | – | – | – |
| UCC | 184.072 | -58.469 | 0.2 | -6.185 | 0.766 | 6.04 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.416, distance=1298, log_age=9.11 |
Search coordinates in Bayestar19